pith:PWAYIGZU
Equilibrium figure of Haumea and possible detection by stellar occultation
Haumea's observed shape matches hydrostatic models near critical rotation that pinch and deviate up to 110 km from an ellipsoid.
arxiv:2603.11787 v2 · 2026-03-12 · astro-ph.EP
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Claims
Using the code BALEINES, which solves for the equilibrium figures of the boundaries between layers, we show that the hydrostatic models closest to the shape derived by stellar occultation approach a state of critical rotation, which translates into a pinched shape with large deviations from an ellipsoid (up to 110 km).
The assumption of three specific interior model groups with a rocky core, an intermediate layer of suggested partial differentiation or organic matter, and a volatile-rich outer shell possibly containing porosity, combined with the premise that Haumea is in hydrostatic equilibrium.
Hydrostatic equilibrium models of Haumea with layered interiors predict a pinched shape deviating up to 110 km from an ellipsoid, potentially detectable in the 2026 occultation.
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Receipt and verification
| First computed | 2026-05-27T14:06:41.508982Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
7d81841b347ebc9538ad8d8fff1ee8e2af406d4e88fcfd86129c079204c783a1
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Canonical record JSON
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